On the possibility of detecting ultra-short period exoplanets with LISA
Autor: | Wong, Kaze W. K., Berti, Emanuele, Gabella, William E., Holley-Bockelmann, Kelly |
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Rok vydání: | 2018 |
Předmět: | |
Druh dokumentu: | Working Paper |
DOI: | 10.1093/mnrasl/sly208 |
Popis: | Cunha et al. (2018) recently reexamined the possibility of detecting gravitational waves from exoplanets, claiming that three ultra-short period systems would be observable by LISA. We revisit their analysis and conclude that the currently known exoplanetary systems are unlikely to be detectable, even assuming a LISA observation time $T_{\rm obs}=4$ yrs. Conclusive statements on the detectability of one of these systems, GP Com b, will require better knowledge of the system's properties, as well as more careful modeling of both LISA's response and the galactic confusion noise. Still, the possibility of exoplanet detection with LISA is interesting enough to warrant further study, as gravitational waves could yield dynamical properties that are difficult to constrain with electromagnetic observations. Comment: 4 pages, 1 figure, 2 tables, revised in response to referee's comments and accepted in MNRAS |
Databáze: | arXiv |
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